Lecture #7

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Lecture #7 What makes a good eye? Part I. Resolution Land and Nilsson first half of chapter 3 2/14/13

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Lecture #7. What makes a good eye? Part I. Resolution Land and Nilsson first half of chapter 3 2 /14/13. Two key features of an eye. Resolution (today) Precision with which eye can resolve or distinguish a spatial image Sensitivity (next time) How much light can be detected by the eye. - PowerPoint PPT Presentation

Transcript of Lecture #7

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Lecture #7

What makes a good eye? Part I. Resolution

Land and Nilsson first half of chapter 3

2/14/13

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Two key features of an eye

• Resolution (today)Precision with which eye can resolve

or distinguish a spatial image

• Sensitivity (next time)How much light can be detected by the

eye

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Eye design

• Optical devices are subject to laws of physics and optimized by the engineers who design them

• Eyes are subject to laws of physics and optimized by evolution

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Camera - transfers object image to “film”

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Image resolution depends on pixel density

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Vertebrate eye - single lens which transfers image to retina

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Spatial resolution depends on cone spacing

Wolfe et al Sensory Perception fig 2.9

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Human retinal mosaic in foveaJW temporal nasal AN nasal

Roorda and Williams 1999

Huge variation from person to person in distribution of cones and in M/L cone ratios!

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Optimizing resolution

• Receptor size and spacing

• Lens focal length

• Optical imperfections

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YouAreHere

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v v

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v

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High Resolution Low Resolution

Why does this even exist?

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Resolution - seeing one point of light

receptor

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Reasons that points of light might end up as blurred points

of light

• Lens does not focus perfectlyAberration = imperfection

• Cornea, lens or humours scatter some of light

• DiffractionWhen light goes through an aperture,

it gets diffracted

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Resolution

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Optimal receptor spacing to resolve objects

• Need enough photoreceptors to define boundaries between objects

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Optimal receptor spacing

• If receptors are too big (spaced too coarsely) they can’t resolve fine detail

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Want optimal receptor spacing• No reason to have more receptors than this as

they won’t resolve the images any better

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Refraction: Light bends at interface

More dense

Less dense

Bigger incident angle = more bending

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Lens focal length, f

• Focal length is distance at which parallel light is focused

f

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Lens focal length

• Determined by curvature of lens surface

Lens radius of curvature

Curvature as if cut lens out of surface of sphere with that radius

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Lens focal length

• Determined by curvature of lens surface

Radius of curvature of sphere that matches lens’s curvature

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Lens focal length is determined by curvature of lens surfaces

Large radius of curvature =

large focal length

Small radius of curvature =

small focal length

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Calculate focal length from lens makers equation

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Lens focal length

• Determined by curvature of lens surface

For thin lens

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Lens focal length

If lens is symmetric, R1=-R2=R

If lens is flat on one side, R2=∞

How can we make focal length longer?

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PhET lens simulator

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Physics lens equation

Distance of image and object in relation to lens focal length

dO

Object Image

di

f

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Physics lens equation

If dO, object distance is very large dO>>di

dO

O I

di

So di = f

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Principal rays and nodal point

dO di

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Note: both cornea and lens focus the light so retina is

located at combined focal length of lens and cornea

Retina

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Eye resolution

Determine resolution based on how well can resolve a periodic pattern or grating

One period of grating

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Quantifying resolution

• Minimum resolvable grating will match receptor spacing

• If receptor spacing is s then grating covers 2s on retina

• Angle = 2s / f

f

Angle

2s

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One cycle of grating covers two photoreceptors

• Angle = 2s / f

• So can resolve one cycle if it covers no less than that angle

• Max resolvable spatial frequencyv = 1 / angle of one

grating cycle = f / 2s

s

f

Angle

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Angles

retina

grating

2s

f

θTanθ= 2s / fBut for small θ tanθ=θSo θ= 2s/f

θ is in radians!

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Interreceptor angle

Angle between two adjacent photoreceptors

θ = s / f

s

f

Angleθ

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One cycle of grating covers two photoreceptors

• To cover full cycle of grating the angle is 2θ= 2s / f

• Maximum resolvable spatial frequency, vv = 1/2θ= f / 2s

s

f

Angle2θ

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Minimum receptor acceptance angle

• Another angle:Δρ minimum

receptor acceptance angle

f eye focal length = distance to retina

d receptor diameter

Resolution =1/ Δρ = f/d

Δρ

f

d

In general s ≈ d and 2s/f ≈ 2d/f

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Two ways to characterize eye resolution

• Maximum resolvable spatial frequency, v = f/2s

sf

Angle2θ=2s/f

Δρ

fd

Inter-receptor spacing, Δρ = d/f

Grating resolution = f / 2s Receptor resol = 1/Δρ= f/d = f /s

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Some typical spatial frequencies - Vertebrate eyes

Animal Max resolvable spatial freq

Inter-receptor angle

Eagle 8000 cycles/rad

0.0036 deg

Human 4175 0.007

Cat 573 0.05

Goldfish 409 0.07

Rat 57 0.5

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Some typical spatial frequencies - Vertebrate eyes

Animal Max resolvable spatial freq

Inter-receptor angle, Δρ

Eagle 8000 cycles/rad

0.0036 deg

Human 4175 0.007

Cat 573 0.05

Goldfish 409 0.07

Rat 57 0.5

Δρ= 0.0036º * π / 180 º = 6.28 x 10-5 rad

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Some typical spatial frequencies - Vertebrate eyes

Animal Max resolvable spatial freq

Inter-receptor angle, Δρ

Eagle 8000 cycles/rad

0.0036 deg

Human 4175 0.007

Cat 573 0.05

Goldfish 409 0.07

Rat 57 0.5

Δρ= 0.0036º * π / 180 º = 6.28 x 10-5 rad

v = 1 / 2Δρ = 1 / (2*6.28 x 10-5) = 7960 cycles / rad

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WHAT ABOUT ME?

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How can we modify an eye to get highacuity night vision?

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Chicken Owl

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Image size relative to object size: Similar triangles

• f is focal length of the eye

• O = object size• I = image size

• U=distance to object

• O / U = I / f

f

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Image size relative to object size: Similar triangles

• O / U = I / f

• f is focal length of the eye

• O = object size• I = image size

• U=distance to object

O

I

U

f

Magnification = I / O = f / U

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PhET lens simulator

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Spatial frequency = cycles per degree

Spatial frequency Eye resolution

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Resolvable spatial frequency = f / 2s

• How can we make spatial frequency and therefore eye resolution increase?

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Increasing eye resolution

• Spatial freq = resolution = f / 2s

• Decrease receptor size, sCan’t decrease below 2 μm Smaller receptors leak light

• Increase lens focal length, f

sf

Angle

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What happens as f gets bigger?

• O / U = I / f

• O and U stay same

• What happens to I as f gets bigger?

f• If s stays the same, what happens?

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Lens

• To increase resolution increase lens focal length, f

• Retina needs to be at a distance f from the focusing elements (lens / cornea combo)

• To increase f, what does this require?

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Some typical spatial frequencies - Vertebrate eyes

Animal Max resolvable spatial freq

Inter-receptor angle

Eagle 8000 cycles/rad

0.0036 deg

Human 4175 0.007

Cat 573 0.05

Goldfish 409 0.07

Rat 57 0.5

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Some typical spatial resolutions - Invert eyes

Animal Max resolvable spatial freq

Inter-receptor angle

Octopus 2632 cycles/rad

0.011 deg

Jumping spider 716 0.04

Worker bee 30 0.95

Crab 19 1.5

Drosophila 5.7 5

Nautilus 3.6 8

Flatworm 0.8 35

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T

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Rule of “thumb”

• If you view your thumb at arms length, it subtends about 2 degrees

• Human resolution is 4000 cycles / radSince π radians = 180 degreesThis is 73 cycles / deg

• So you can resolve 146 cycles across your thumb

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Eye chart

Further down chart you can read, the better your visual acuity

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Eye chart is based on sine gratings

1700 cycles / radian

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Typical human spatial acuity

• Can resolve <0.01 deg

• Place letters at 20 ft

• Visual acuity = Resolution you have at 20

ft Distance at which

“normal” viewer would have same resolution as you

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Limitations to eye resolution

• Diffraction• Optical aberrations

SphericalChromatic

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Diffraction

• When light passes through an aperture or lens, it will be distorted by diffraction

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Diffraction

• When light passes through a lens, it will be distorted by diffraction

Edges do not slow down as much as middleWhen arrive at retina, the edge and middle interfere

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Diffraction

• Along center line will constructively interfere

• On sides, will destructively interfere

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Diffraction

• Airy disk - width of interference peak is w = λ / D

D w

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Calculate w two ways and compare

• λ = 650 nm (red laser) • D = 0.088 mm

Spot widthdistance

w= spot width / distance = 1 inch / 17 ft * 12 inch/ft

= 0.005 rad not too bad compared to expectation

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Diffraction through aperture

• Distance from bright to first dark spot

Sin θ = λ / Dλ = wavelengthD = slit width

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What does this mean for humans

• Pupil diameter = 2 mm• Visible light λ = 500 nm

Spatial frequency = 1/wSo humans can resolve 1/.00025

radians or about 4000 cycles / radian

Diffraction limit

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Resolution of human cones in fovea

Cone diameter 2 μm2 s = 4 μmDistance 20 mm

Angle = 2s/f = 4 μm / 20mm

= 0.0002 rad

= 0.011°

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Resolution of human cones in fovea

• Angular resolution based on cone spacing0.0002 rad or 0.011°

• Spatial frequency = 1/angular resolution5000 cycles / rad or 90 / deg

• Diffraction limit4000 cycles /radSo cone spacing is close to diffraction limit

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Diffraction Spatial frequency = 1/w = D / λ

• How does an eagle see 8000 cycles / rad

• What has to change so it has better resolution (and overcomes diffraction?)

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Imperfections in the visual system

• Diffraction when light goes through aperture

• Several other defects of lens systems

Fig 3.6

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Optical defects 1. Lens focal defect

• Myopia

• Near sighted

• Cornea / lens focus too much

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Optical defects 1. Lens focal defect

• Hyperopia

• Far sighted

• Cornea / lens focus not enough

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2. Lens spherical aberration

• Light at edges is bent more than light in center of lens

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2. Lens spherical aberration

• Light at edges is bent more than light in center of lens

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3. Lens chromatic aberration

• Lens index of refraction and so focal length varies with wavelength • Light of different wavelengths are

focused to different points

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Refraction as function of wavelength

λ n2 f

440 1.4155 12.03 cm486 1.410 12.19590 1.4015 12.45650 1.3983 12.55

Blue light bends moreWill focus in front of red light

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Human lens index of refractionVaries between edge and center - correct for aberrations

Sivak and Mandelman 1982

Center inner outer periphery

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Spherical aberration of human lens

1.386

1.406

Periphery focuses less than in center to exactly compensate for spherical aberration